The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. ex. Some numerals are expressed as "XNUMX".
Copyrights notice
The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. Copyrights notice
조회수
87
이 문서에서는 장치 관점에서 ALMA(Atacama Large Millimeter/Submillimeter Array)용 초전도체-절연체-초전도체(SIS) 믹서 개발에 대해 설명합니다. ALMA 건설 단계에서 일본국립천문대(NAOJ)는 대역 230(5~10GHz)에 대해 787K(양자 잡음의 950배) 미만이라는 엄격한 ALMA 잡음 온도 요구 사항을 충족하는 SIS 믹서를 성공적으로 제작했습니다. 국립정보통신기술원과 협력. 밴드 10은 ALMA의 최고 주파수 대역을 커버하며 초전도 기술 측면에서 가장 어려운 대역으로 인식된다. 건설 후 NAOJ는 제시된 최고 수준의 과학 요구 사항에 따라 광대역 및 다중 빔 SIS 믹서와 같은 ALMA 향상을 위한 개발 연구를 시작했습니다.
Yoshinori UZAWA
NAOJ
Matthias KROUG
UBC
Takafumi KOJIMA
NAOJ
Masanori TAKEDA
Shizuoka Univ.
Kazumasa MAKISE
AIST
Shohei EZAKI
NAOJ
Wenlei SHAN
NAOJ
Akihira MIYACHI
NAOJ
Yasunori FUJII
NAOJ
Hirotaka TERAI
NICT
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부
Yoshinori UZAWA, Matthias KROUG, Takafumi KOJIMA, Masanori TAKEDA, Kazumasa MAKISE, Shohei EZAKI, Wenlei SHAN, Akihira MIYACHI, Yasunori FUJII, Hirotaka TERAI, "Development of Superconducting Devices Supporting Radio Astronomy" in IEICE TRANSACTIONS on Electronics,
vol. E104-C, no. 9, pp. 411-421, September 2021, doi: 10.1587/transele.2020SUI0003.
Abstract: This paper describes the development of superconductor-insulator-superconductor (SIS) mixers for the Atacama Large Millimeter/submillimeter Array (ALMA) from the device point of view. During the construction phase of ALMA, the National Astronomical Observatory of Japan (NAOJ) successfully fabricated SIS mixers to meet the stringent ALMA noise temperature requirements of less than 230 K (5 times the quantum noise) for Band 10 (787-950 GHz) in collaboration with the National Institute of Information and Communications Technology. Band 10 covers the highest frequency band of ALMA and is recognized as the most difficult band in terms of superconducting technology. After the construction, the NAOJ began development studies for ALMA enhancement such as wideband and multibeam SIS mixers according to top-level science requirements, which are also presented.
URL: https://global.ieice.org/en_transactions/electronics/10.1587/transele.2020SUI0003/_p
부
@ARTICLE{e104-c_9_411,
author={Yoshinori UZAWA, Matthias KROUG, Takafumi KOJIMA, Masanori TAKEDA, Kazumasa MAKISE, Shohei EZAKI, Wenlei SHAN, Akihira MIYACHI, Yasunori FUJII, Hirotaka TERAI, },
journal={IEICE TRANSACTIONS on Electronics},
title={Development of Superconducting Devices Supporting Radio Astronomy},
year={2021},
volume={E104-C},
number={9},
pages={411-421},
abstract={This paper describes the development of superconductor-insulator-superconductor (SIS) mixers for the Atacama Large Millimeter/submillimeter Array (ALMA) from the device point of view. During the construction phase of ALMA, the National Astronomical Observatory of Japan (NAOJ) successfully fabricated SIS mixers to meet the stringent ALMA noise temperature requirements of less than 230 K (5 times the quantum noise) for Band 10 (787-950 GHz) in collaboration with the National Institute of Information and Communications Technology. Band 10 covers the highest frequency band of ALMA and is recognized as the most difficult band in terms of superconducting technology. After the construction, the NAOJ began development studies for ALMA enhancement such as wideband and multibeam SIS mixers according to top-level science requirements, which are also presented.},
keywords={},
doi={10.1587/transele.2020SUI0003},
ISSN={1745-1353},
month={September},}
부
TY - JOUR
TI - Development of Superconducting Devices Supporting Radio Astronomy
T2 - IEICE TRANSACTIONS on Electronics
SP - 411
EP - 421
AU - Yoshinori UZAWA
AU - Matthias KROUG
AU - Takafumi KOJIMA
AU - Masanori TAKEDA
AU - Kazumasa MAKISE
AU - Shohei EZAKI
AU - Wenlei SHAN
AU - Akihira MIYACHI
AU - Yasunori FUJII
AU - Hirotaka TERAI
PY - 2021
DO - 10.1587/transele.2020SUI0003
JO - IEICE TRANSACTIONS on Electronics
SN - 1745-1353
VL - E104-C
IS - 9
JA - IEICE TRANSACTIONS on Electronics
Y1 - September 2021
AB - This paper describes the development of superconductor-insulator-superconductor (SIS) mixers for the Atacama Large Millimeter/submillimeter Array (ALMA) from the device point of view. During the construction phase of ALMA, the National Astronomical Observatory of Japan (NAOJ) successfully fabricated SIS mixers to meet the stringent ALMA noise temperature requirements of less than 230 K (5 times the quantum noise) for Band 10 (787-950 GHz) in collaboration with the National Institute of Information and Communications Technology. Band 10 covers the highest frequency band of ALMA and is recognized as the most difficult band in terms of superconducting technology. After the construction, the NAOJ began development studies for ALMA enhancement such as wideband and multibeam SIS mixers according to top-level science requirements, which are also presented.
ER -